LP 788-1 , the SIMBAD biblio

LP 788-1 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST12:33:23

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2003A&A...401..959P viz 148 40 New neighbours. V. 35 DENIS late-M dwarfs between 10 and 30 parsecs. PHAN-BAO N., CRIFO F., DELFOSSE X., et al.
2005A&A...441..653C viz 70 30 New neighbours. VI. Spectroscopy of DENIS nearby stars candidates. CRIFO F., PHAN-BAO N., DELFOSSE X., et al.
2007A&A...468..163D viz 15       D   O           1 7019 33 Southern infrared proper motion survey. II. A sample of low mass stars with µ≥0.1"/yr. DEACON N.R. and HAMBLY N.C.
2012ApJ...746...23M viz 15       D               2 242 93 The radio activity-rotation relation of ultracool dwarfs. McLEAN M., BERGER E. and REINERS A.
2013A&A...556A..15R viz 15       D               2 160 185 The effective temperature scale of M dwarfs. RAJPUROHIT A.S., REYLE C., ALLARD F., et al.
2015AJ....149....5W viz 16       D               1 1773 104 The solar neighborhood. XXXV. Distances to 1404 M dwarf systems within 25 pc in the southern sky. WINTERS J.G., HAMBLY N.C., JAO W.-C., et al.
2016ApJ...817..112S viz 16       D               1 20555 25 A proper motion survey using the first sky pass of NEOWISE-reactivation data. SCHNEIDER A.C., GRECO J., CUSHING M.C., et al.
2017AJ....153...14W viz 254       D     X C       6 161 11 The solar neighborhood XXXVIII. Results from the CTIO/SMARTS 0.9M: trigonometric parallaxes for 151 nearby M dwarf systems. WINTERS J.G., SEVRINSKY R.A., JAO W.-C., et al.
2018AJ....156..217N viz 16       D               1 580 80 New rotation period measurements for M dwarfs in the southern hemisphere: an abundance of slowly rotating, fully convective stars. NEWTON E.R., MONDRIK N., IRWIN J., et al.
2020A&A...634A.128N 82               F     2 90 ~ Sporadic and intense accretion in a 1 Myr-old brown dwarf candidate. NGUYEN-THANH D., PHAN-BAO N., MURPHY S.J., et al.
2020A&A...637A..45S 16       D               1 82 ~ New ultracool dwarf neighbours within 20 pc from Gaia DR2. SCHOLZ R.-D.
2020AJ....160..215V viz 16       D               1 605 16 The solar neighborhood. XLVI. Revealing new M dwarf binaries and their orbital architectures. VRIJMOET E.H., HENRY T.J., JAO W.-C., et al.
2021A&A...645A.100S viz 17       D               1 1696 44 SPECULOOS: Ultracool dwarf transit survey. Target list and strategy. SEBASTIAN D., GILLON M., DUCROT E., et al.
2021AJ....161...63W viz 17       D               1 574 22 The volume-complete sample of M dwarfs with masses 0.1 <= M/M☉ <= 0.3 within 15 parsecs. WINTERS J.G., CHARBONNEAU D., HENRY T.J., et al.
2021A&A...649A...6G viz 17       D               1 227180 168 Gaia Early Data Release 3. The Gaia Catalogue of Nearby Stars. GAIA COLLABORATION, SMART R.L., SARRO L.M., et al.
2022AJ....163..178V viz 85           X         2 38 9 The Solar Neighborhood. XLIX. New Discoveries and Orbits of M-dwarf Multiples with Speckle Interferometry at SOAR. VRIJMOET E.H., TOKOVININ A., HENRY T.J., et al.
2022MNRAS.513.2615M viz 17       D               1 159 7 A study of flares in the ultra-cool regime from SPECULOOS-South. MURRAY C.A., QUELOZ D., GILLON M., et al.
2023A&A...670A..19G viz 17       D               1 5915 6 The Fifth Catalogue of Nearby Stars (CNS5). GOLOVIN A., REFFERT S., JUST A., et al.
2023AJ....165..265M viz 17       D               1 332 5 The Occurrence Rate of Terrestrial Planets Orbiting Nearby Mid-to-late M Dwarfs from TESS Sectors 1-42. MENT K. and CHARBONNEAU D.
2023AJ....165..267H viz 17       D               1 64663 1 Bioverse: A Comprehensive Assessment of the Capabilities of Extremely Large Telescopes to Probe Earth-like O2 Levels in Nearby Transiting Habitable-zone Exoplanets. HARDEGREE-ULLMAN K.K., APAI D., BERGSTEN G.J., et al.
2024AJ....167...56C viz 18       D               1 1125 ~ The POKEMON Speckle Survey of Nearby M Dwarfs. II. Observations of 1125 Targets. CLARK C.A., VAN BELLE G.T., HORCH E.P., et al.

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